百度试题 结果1 题目〔 〕The temperature on Mars changes a lot in a day.相关知识点: 试题来源: 解析 Could can’t 反馈 收藏
On Mars,the temperature is about -60℃.So one of the main purposes is to warm it up.One idea for warming Mars comes from a problem here on Earth-climate(气候)change.Most scientists agree that Earth is becoming warmer because of increased levels of greenhouse gases(大气).We might create ...
Then how can we make Mars a right place for humans to live on? The answer is to change the environment of the planet so that it is similar to Earth’s. On Mars, the temperature is about —60℃. So one of the main purposes is to warm it up. One idea for warming Mars comes ...
So how can we make Mars inhabitable? The answer is a process called terraforming. Terraforming means changing the environment of a planet so that it is similar to Earth’s. On Mars, the average temperature is about -60 degrees Celsius. So one of the main goals of terraforming Mars is to...
The temperature on Mars is between -140℃ and 30℃. At the north and south poles (极) of Mars, there are areas covered by ice and snow. There is also a big mountain called Olympus. So maybe we can ski on Mars! Pluto (冥王星) is a small planet far away from the sun. It’s ...
根据“In the daytime, the temperature can be up to 430℃ but at night it cools down to -200℃.”可知水星上最低温度为零下200度。故选B。 (2)题详解: 细节理解题。根据“There is also a big mountain called Mount Olympus, So maybe we can ski on Mars!”可知我们可能在火星上滑雪。故选A...
the heat flow at the north polar region, we use the lower limit of the effective elastic thickness of the lithosphere loaded by the north polar cap, crustal heat-producing elements (HPE) abundances based on martian geochemistry, and a temperature-dependent thermal conductivity for the upper ...
July, the storm had died down, but then grew again to become the largest storm in 25 years. So big was the storm that amateur astronomers using small telescopes were able to see it from Earth. And the cloud raised the temperature of the frigid Martian atmosphere by a stunning 30° ...
We calculate the temperature profile following the procedure described by Ruiz et al.8,15, and using crustal heat-producing elements (HPE) abundances based on Mars Odyssey GRS measurements (see above). We perform this calculation using a Cartesian geometry, because it is sufficient for deriving ...
(b) The temperature profiles obtained by MAVEN in the Non-Crustal Field (NCF) and Crustal Field (CF) regions on Mars [121]. 4 相关问题讨论 4.1 MB分布的适用性 虽然金斯逃逸在概念上非常简单, 但针对逃逸面处的粒子速度分布函数是否满足MB分布, 依然存在一些悬而未决的争论, 简述如下. 其一, ...